Niobium-zirconium chronometry and early solar system development.
Niobium-92 (92Nb) decays to zirconium-92 (92Zr) with a half-life of 36 million years and can be used to place constraints on the site of p-process nucleosynthesis and the timing of early solar system processes. Recent results have suggested that the initial 92Nb/93Nb of the solar system was high (&a...
المؤلفون الرئيسيون: | Schönbächler, M, Rehkämper, M, Halliday, A, Lee, D, Bourot-Denise, M, Zanda, B, Hattendorf, B, Günther, D |
---|---|
التنسيق: | Journal article |
اللغة: | English |
منشور في: |
2002
|
مواد مشابهة
-
Zirconium isotope evidence for incomplete admixing of r-process components in the solar nebula
حسب: Schonbachler, M, وآخرون
منشور في: (2003) -
Nucleosynthetic zirconium isotope anomalies in acid leachates of carbonaceous chondrites
حسب: Schonbachler, M, وآخرون
منشور في: (2005) -
Hf-182-W-182 chronometry for Renazzo and Bencubbinites
حسب: Lee, D, وآخرون
منشور في: (2002) -
Zirconium isotopes in carbonaceous chondrites
حسب: Schonbachler, M, وآخرون
منشور في: (2003) -
Ion exchange chromatography and high precision isotopic measurements of zirconium by MC-ICP-MS
حسب: Schonbachler, M, وآخرون
منشور في: (2004)